[1]} presented FIP and TIP testing as good practice for the analysis of RV data, given that assumptions on the priors and the noise model (log\(\cal {L}\) ) might be incorrect. Following this idea, we searched for various planets simultaneously using a frequency window sliding along the entire frequency space spanned by the posterior distribution of the 2-planet model (with CoRoT-7b being known). Consequently, two strong peaks were found, at 3.697 days and 8.965 days, both with significantly minimal FIP and maximal TIP, reinforcing their planetary nature (Figure REF ). To avoid being misled by the shared power among adjacent interference peaks linked with relevant signals, a basic histogram was used to find these most probable periods, See Figure REF .
